Dear Colleagues,
This is the second announcement for the 14th European Solar Physics
Meeting (ESPM-14) that will take place in Dublin, Ireland over 8-12
September 2014. The meeting will be hosted by Trinity College Dublin,
which is centrally located in Dublin city. ESPMs are organized by the
Board of the European Solar Physics Division (ESPD), a joint Division
of the European Physical Society (EPS) and the European Astronomical
Society (EAS). These meetings occur every 3 years with the purpose of
bringing together researchers from Europe and beyond that are active
in the theoretical and observational study of all solar phenomena.
We are pleased to announce the following preliminary list of science
session titles for ESPM-14:
Session 1 - New and Upcoming Heliospheric Observational and Data Assimilation Facilities
Session 2 - The Sun as a Whole: Large-Scale Flows, Magnetism, Magnetoconvection and the Solar Cycle
Session 3 - Emergence and Evolution of Magnetic Flux in the Solar Atmosphere
Session 4 - Chromospheric Dynamics
Session 5 - Heating and Transient Activity of the Solar Corona: Waves, Flows, Reconnection and Jets
Session 6 - Solar Eruptive Events: Instabilities, Flares and Coronal Mass Ejections
Session 7 - Radio Emission and Particle Acceleration
Session 8 - The Solar Wind and Space Weather Research
Online registration and abstract submission will open in early spring
2014. The ESPM-14 Local and Scientific Organizing Committees are
currently working to secure funding that will provide financial aid
to a number of PhD students via partial travel and/or local support.
Further details related to registration costs, abstract submission,
accomodation, financial assistance and relevant deadlines will be
circulated in a third announcement shortly after the New Year.
The meeting website can be found at http://www.espm14.ie
We look forward to welcoming you to Dublin.
Best regards,
ESPM-14 Scientific and Local Organizing Committees
Dear all,
We are pleased to announce the release of a new EIS nugget by Jeff Brosius entitled: 'Rapid Evolution of the Solar Atmosphere During a Microflare Observed with EIS: Hints of Chromospheric Magnetic Reconnection'.
The nugget can be found here:
http://solarb.mssl.ucl.ac.uk/SolarB/nuggets/nugget_2013nov.jsp
We welcome nugget contributions from the community. Please contact Deb Baker or Lucie Green if you are interested.
Best wishes,
Deb Baker
--
Dr. Deb Baker
UCL - Mullard Space Science Laboratory
Email: Deborah.Baker(a)ucl.ac.uk
Tel: +44 (0) 1483 204 179
MAX MILLENNIUM NEWS
30 October 2013
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Homologous Flux Ropes Observed by SDO/AIA
-- Ting Li & Jun Zhang
The dynamical behaviour of a jet in an on-disk coronal hole observed
with AIA/SDO
-- K. Chandrashekhar, R. J. Morton, D. Banerjee and G. R. Gupta
Evidence of Multiple Slow Acoustic Oscillations in the Stellar
Flaring Loops of Proxima Centauri
-- Srivastava, A. K.; Lalitha, S.; Pandey, J. C.
Tracking the Evolution of A Coherent Magnetic Flux Rope Continuously
from the Inner to the Outer Corona
-- X. Cheng, M. D. Ding, Y. Guo, J. Zhang, A. Vourlidas, Y. D. Liu,
O. Olmedo, J. Q. Sun, and C. Li
2. FROM THE EDITOR ------------------
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu
MAX MILLENNIUM NEWS
23 October 2013
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Time-Dependent Modulation of Cosmic Rays in the Heliosphere
-- Manuel, R., Ferreira, S. E. S., Potgieter, M. S.
Evidence for Solar Tether-cutting Magnetic Reconnection from Coronal
Field Extrapolations
-- Chang Liu, Na Deng, Jeongwoo Lee, Thomas Wiegelmann, Ronald
L. Moore, and Haimin Wang
Variation of proton flux profiles with the observer's latitude
in simulated gradual SEP events
-- R. Rodriguez-Gasen, A. Aran, B. Sanahuja, C. Jacobs, S. Poedts
Imaging of the solar atmosphere by the Siberian Solar Radio Telescope
at 5.7 GHz with an enhanced dynamic range
-- Alexey Kochanov, Sergey Anfinogentov, Dmitry Prosovetsky, George
Rudenko, Victor Grechnev
2. FROM THE EDITOR ------------------
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu
MAX MILLENNIUM NEWS
16 October 2013
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
On the sensitivity of the GOES flare classification to properties
of the electron beam in the thick target model
-- Reep, J.W., Bradshaw, S.J., McAteer R.T.J.
Electron Distribution Functions in Solar Flares from combined X-ray
and EUV Observations
-- Marina Battaglia & Eduard P. Kontar
A Macroscopic Description of Self-Organized Criticality Systems
and Astrophysical Applications
-- Markus J. Aschwanden
3D Reconstruction of Coronal Loops by the Principal Component
Analysis
-- Giuseppe Nistico, Erwin Verwichte, Valery M. Nakariakov
Quasiperiodic acceleration of electrons by a plasmoid-driven shock
in the solar atmosphere
-- Eoin P. Carley, David M. Long, Jason P. Byrne, Pietro Zucca,
D. Shaun Bloomfield, Joseph McCauley and Peter T. Gallagher
2. FROM THE EDITOR ------------------
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu
MAX MILLENNIUM NEWS
09 October 2013
CONTENTS
1. MMSCIENCE AND THE SOLAR PHYSICS E-PRINT ARCHIVE: A MILESTONE
2. E-PRINTS POSTED IN THE PAST WEEK
3. FROM THE EDITOR
=====================================================================
1. MMSCIENCE AND THE SOLAR PHYSICS E-PRINT ARCHIVE: A MILESTONE
----------------------------------------------
> From the Editor
This issue of Max Millennium News is the 1000th mail message be sent
to all subscribers to MMscience, the Max Millennium Science mailing
list, presently numbering about 400 worldwide. Max Millennium
News is the voice of the Solar Physics E-Print Archive, which for
the past 15 years has been maintained by Dr. Alisdair Davey, as
a pro bono service to the scientific community. Please join me in
thanking Alisdair for his enduring contribution to our discipline.
2. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Hot Spine Loops and the Nature of a Late-Phase Solar Flare
-- Xudong Sun, J. Todd Hoeksema, Yang Liu, Guillaume Aulanier,
Yingna Su, Iain G. Hannah, Rachel A. Hock
Emission Height and Temperature Distribution of White-Light Emission
Observed by Hinode/SOT from the 2012 January 27 X-class Solar Flare
-- Kyoko Watanabe, Toshifumi Shimizu, Satoshi Masuda, Kiyoshi Ichimoto,
and Masanori Ohno
Fragmentation of electric currents in the solar corona by plasma
flows
-- Nickeler, D. H., Karlicky, M., Wiegelmann, T., Kraus, M.
Flare line impact polarization. Na D2 589 nm line polarization in
the 2001 June 15 flare
-- Henoux, J.C., Karlicky, M.
Self-assembly of shallow magnetic spots through strongly stratified
turbulence
-- Axel Brandenburg, Nathan Kleeorin, Igor Rogachevskii
Plasma composition of a sigmoidal anemone active region
-- D. Baker, D. H. Brooks, P. Demoulin, L. Gesztelyi, L. M. Green,
J. Carlyle
A confined flare above filaments
-- K. Dalmasse, R. Chandra, B. Schmieder and G. Aulanier
2. FROM THE EDITOR ------------------
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu
Dear all,
We are pleased to announce the release of a new EIS nugget by S. Imada, K. Aoki, H. Hara, T. Watanabe, L. K. Harra, and T. Shimizu. This month's nugget is entitled: "Clear evidence for hot fast flows above a solar flare arcade".
Please visit the nugget here:
http://solarb.mssl.ucl.ac.uk/SolarB/eisnuggets.jsp
We welcome nugget contributions from the community. Please contact Deb Baker or Lucie Green if you are interested.
Best wishes,
Deb Baker
--
Dr. Deb Baker
UCL - Mullard Space Science Laboratory
Email: Deborah.Baker(a)ucl.ac.uk
Tel: +44 (0) 1483 204 179
MAX MILLENNIUM NEWS
02 Octobeer 2013
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Magnetoacoustic waves in a partially ionized two-fluid plasma
-- R. Soler, M. Carbonell, J. L. Ballester
The physical mechanisms that initiate and drive solar eruptions
-- Aulanier G.
First magnetic seismology of the CME reconnection outflow layer in
the low corona with 2.5-D MHD simulations of the Kelvin-Helmholtz
instability
== Nykyri, K. and Foullon, C.
Kelvin-Helmholtz Instability of the CME Reconnection Outflow Layer in
the Low Corona
-- Foullon, C., Verwichte, E., Nykyri, K., Aschwanden, M.J., Hannah, I. G.
2. FROM THE EDITOR ------------------
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu